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The contribution of...
The contribution of the ARIEL space mission to the study of planetary formation
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- Turrini, D. (författare)
- University of Atacama,Institute for Space Astrophysics and Planetology
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- Miguel, Y. (författare)
- Leiden University
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- Zingales, T. (författare)
- INAF Palermo Astronomical Observatory,University College London
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- Piccialli, A. (författare)
- Belgian Institute for Space Aeronomy
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- Helled, R. (författare)
- University of Zurich
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- Vazan, A. (författare)
- University of Amsterdam
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- Oliva, F. (författare)
- Institute for Space Astrophysics and Planetology
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- Sindoni, G. (författare)
- Institute for Space Astrophysics and Planetology
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- Panić, O. (författare)
- University of Leeds
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- Leconte, J. (författare)
- Bordeaux Observatory
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- Min, M. (författare)
- University of Amsterdam
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- Pirani, S. (författare)
- Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
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- Selsis, F. (författare)
- Bordeaux Observatory
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- Coudé du Foresto, V. (författare)
- Paris Observatory
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- Mura, A. (författare)
- Institute for Space Astrophysics and Planetology
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- Wolkenberg, P. (författare)
- Institute for Space Astrophysics and Planetology,Space Research Centre
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(creator_code:org_t)
- 2018-01-29
- 2018
- Engelska.
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Ingår i: Experimental Astronomy. - : Springer Science and Business Media LLC. - 0922-6435 .- 1572-9508. ; 46:1, s. 45-65
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Abstract
Ämnesord
Stäng
- The study of extrasolar planets and of the Solar System provides complementary pieces of the mosaic represented by the process of planetary formation. Exoplanets are essential to fully grasp the huge diversity of outcomes that planetary formation and the subsequent evolution of the planetary systems can produce. The orbital and basic physical data we currently possess for the bulk of the exoplanetary population, however, do not provide enough information to break the intrinsic degeneracy of their histories, as different evolutionary tracks can result in the same final configurations. The lessons learned from the Solar System indicate us that the solution to this problem lies in the information contained in the composition of planets. The goal of the Atmospheric Remote-Sensing Infrared Exoplanet Large-survey (ARIEL), one of the three candidates as ESA M4 space mission, is to observe a large and diversified population of transiting planets around a range of host star types to collect information on their atmospheric composition. ARIEL will focus on warm and hot planets to take advantage of their well-mixed atmospheres, which should show minimal condensation and sequestration of high-Z materials and thus reveal their bulk composition across all main cosmochemical elements. In this work we will review the most outstanding open questions concerning the way planets form and the mechanisms that contribute to create habitable environments that the compositional information gathered by ARIEL will allow to tackle.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- ARIEL
- Astrochemistry
- Atmospheric remote-sensing infrared exoplanet large-survey
- Exoplanets
- Planetary formation
- Space missions
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
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Till lärosätets databas
- Av författaren/redakt...
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Turrini, D.
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Miguel, Y.
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Zingales, T.
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Piccialli, A.
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Helled, R.
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Vazan, A.
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visa fler...
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Oliva, F.
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Sindoni, G.
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Panić, O.
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Leconte, J.
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Min, M.
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Pirani, S.
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Selsis, F.
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Coudé du Foresto ...
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Mura, A.
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Wolkenberg, P.
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visa färre...
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